Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/237123 |
Resumo: | The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of ∼9300 deg2 in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg2. The data has been fully calibrated using a new photometric calibration technique suitable for the new generation of wide-field multifilter surveys. This technique consists of a χ2 minimization to fit synthetic stellar templates to already calibrated data from other surveys, eliminating the need for standard stars and reducing the survey duration by ∼15 per cent. We compare the template-predicted and S-PLUS instrumental magnitudesto derive the photometric zero-points(ZPs). We show that these ZPs can be further refined by fitting the stellar templates to the 12 S-PLUS magnitudes, which better constrain the models by adding the narrow-band information. We use the STRIPE82 region to estimate ZP errors, which are 10 mmags for filters J0410, J0430, g,J0515, r,J0660, i,J0861 and z; 15 mmags for filterJ0378; and 25 mmagsfor filters u and J0395. We describe the complete data flow of the S-PLUS/DR2 from observations to the final catalogues and present a brief characterization of the data. We show that, for a minimum signal-to-noise threshold of 5, the photometric depths of the DR2 range from 19.1 to 20.5 mag (measured in Petrosian apertures), depending on the filter. The S-PLUS DR2 can be accessed from the website: https://splus.cloud. |
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Fernandes, Felipe de AlmeidaBonatto, Charles JoseChies-Santos, Ana LeonorHartmann, Eduardo AlbuquerqueOliveira, Claudia Lucia Mendes de2022-04-13T04:51:14Z20220035-8711http://hdl.handle.net/10183/237123001139019The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of ∼9300 deg2 in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg2. The data has been fully calibrated using a new photometric calibration technique suitable for the new generation of wide-field multifilter surveys. This technique consists of a χ2 minimization to fit synthetic stellar templates to already calibrated data from other surveys, eliminating the need for standard stars and reducing the survey duration by ∼15 per cent. We compare the template-predicted and S-PLUS instrumental magnitudesto derive the photometric zero-points(ZPs). We show that these ZPs can be further refined by fitting the stellar templates to the 12 S-PLUS magnitudes, which better constrain the models by adding the narrow-band information. We use the STRIPE82 region to estimate ZP errors, which are 10 mmags for filters J0410, J0430, g,J0515, r,J0660, i,J0861 and z; 15 mmags for filterJ0378; and 25 mmagsfor filters u and J0395. We describe the complete data flow of the S-PLUS/DR2 from observations to the final catalogues and present a brief characterization of the data. We show that, for a minimum signal-to-noise threshold of 5, the photometric depths of the DR2 range from 19.1 to 20.5 mag (measured in Petrosian apertures), depending on the filter. The S-PLUS DR2 can be accessed from the website: https://splus.cloud.application/pdfengMonthly notices of the royal astronomical society. Oxford. Vol. 511, no. 3 (Apr. 2022), p. 4590-4618Fotometria astronômicaCatalogos astronomicosEstrelasGaláxiasTechniques: photometricAstronomical databases: miscellaneousCataloguesSurveysStars: generalGalaxies: generalData release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filtersEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001139019.pdf.txt001139019.pdf.txtExtracted Texttext/plain152851http://www.lume.ufrgs.br/bitstream/10183/237123/2/001139019.pdf.txt39be10cd4fa4253cd341a576fd18ae4eMD52ORIGINAL001139019.pdfTexto completo (inglês)application/pdf7215474http://www.lume.ufrgs.br/bitstream/10183/237123/1/001139019.pdf26aaef9060c6edf3966ae114d7b6fa0cMD5110183/2371232023-07-15 03:27:44.565252oai:www.lume.ufrgs.br:10183/237123Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-15T06:27:44Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
title |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
spellingShingle |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters Fernandes, Felipe de Almeida Fotometria astronômica Catalogos astronomicos Estrelas Galáxias Techniques: photometric Astronomical databases: miscellaneous Catalogues Surveys Stars: general Galaxies: general |
title_short |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
title_full |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
title_fullStr |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
title_full_unstemmed |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
title_sort |
Data release 2 of S-PLUS : accurate template-fitting based photometry covering ∼1000 deg2 in 12 optical filters |
author |
Fernandes, Felipe de Almeida |
author_facet |
Fernandes, Felipe de Almeida Bonatto, Charles Jose Chies-Santos, Ana Leonor Hartmann, Eduardo Albuquerque Oliveira, Claudia Lucia Mendes de |
author_role |
author |
author2 |
Bonatto, Charles Jose Chies-Santos, Ana Leonor Hartmann, Eduardo Albuquerque Oliveira, Claudia Lucia Mendes de |
author2_role |
author author author author |
dc.contributor.author.fl_str_mv |
Fernandes, Felipe de Almeida Bonatto, Charles Jose Chies-Santos, Ana Leonor Hartmann, Eduardo Albuquerque Oliveira, Claudia Lucia Mendes de |
dc.subject.por.fl_str_mv |
Fotometria astronômica Catalogos astronomicos Estrelas Galáxias |
topic |
Fotometria astronômica Catalogos astronomicos Estrelas Galáxias Techniques: photometric Astronomical databases: miscellaneous Catalogues Surveys Stars: general Galaxies: general |
dc.subject.eng.fl_str_mv |
Techniques: photometric Astronomical databases: miscellaneous Catalogues Surveys Stars: general Galaxies: general |
description |
The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of ∼9300 deg2 in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg2. The data has been fully calibrated using a new photometric calibration technique suitable for the new generation of wide-field multifilter surveys. This technique consists of a χ2 minimization to fit synthetic stellar templates to already calibrated data from other surveys, eliminating the need for standard stars and reducing the survey duration by ∼15 per cent. We compare the template-predicted and S-PLUS instrumental magnitudesto derive the photometric zero-points(ZPs). We show that these ZPs can be further refined by fitting the stellar templates to the 12 S-PLUS magnitudes, which better constrain the models by adding the narrow-band information. We use the STRIPE82 region to estimate ZP errors, which are 10 mmags for filters J0410, J0430, g,J0515, r,J0660, i,J0861 and z; 15 mmags for filterJ0378; and 25 mmagsfor filters u and J0395. We describe the complete data flow of the S-PLUS/DR2 from observations to the final catalogues and present a brief characterization of the data. We show that, for a minimum signal-to-noise threshold of 5, the photometric depths of the DR2 range from 19.1 to 20.5 mag (measured in Petrosian apertures), depending on the filter. The S-PLUS DR2 can be accessed from the website: https://splus.cloud. |
publishDate |
2022 |
dc.date.accessioned.fl_str_mv |
2022-04-13T04:51:14Z |
dc.date.issued.fl_str_mv |
2022 |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/237123 |
dc.identifier.issn.pt_BR.fl_str_mv |
0035-8711 |
dc.identifier.nrb.pt_BR.fl_str_mv |
001139019 |
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0035-8711 001139019 |
url |
http://hdl.handle.net/10183/237123 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Monthly notices of the royal astronomical society. Oxford. Vol. 511, no. 3 (Apr. 2022), p. 4590-4618 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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